Gravitational Fields Topic 6 1 Gravitational Force What

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Gravitational Fields Topic 6. 1

Gravitational Fields Topic 6. 1

Gravitational Force � What are the variables that affect the gravitational force on an

Gravitational Force � What are the variables that affect the gravitational force on an object? � It was found (discovered? )that : Compare with: Sir Issac Newton (1642 – 1727) What are the major differences?

Newton’s Law of Universal Gravitation

Newton’s Law of Universal Gravitation

Newton’s law of universal gravitation For large objects like the earth, r is the

Newton’s law of universal gravitation For large objects like the earth, r is the distance to the centre of mass

Calculations using Newton’s law What is the force of attraction between Andrei and Mike?

Calculations using Newton’s law What is the force of attraction between Andrei and Mike? 7. 3 x 10 -8 N 2 m 63 kg ? 70 kg ?

Force of gravity due to earth on Mike? 615 N 63 kg ? (Mike’s

Force of gravity due to earth on Mike? 615 N 63 kg ? (Mike’s weight) R = 6400 km, m = 6 x 1024 kg

Force of gravity due to earth on Michael? F = Gm 1 m 2

Force of gravity due to earth on Michael? F = Gm 1 m 2 = 6. 667 x 10 -11 x 63 x 6 x 1024 = 615 N (= mg) r 2 (6400 x 103)2 In other words, for any planet; g = Gmp r p 2

Gravitational field An area or region where a mass feels a gravitational force is

Gravitational field An area or region where a mass feels a gravitational force is called a gravitational field. The gravitational field strength at any point in space is defined as the force per unit mass (on a small test mass) at that point. g = F/m (in N. kg-1)

Gravitational field around a point mass If we have two masses m 1 and

Gravitational field around a point mass If we have two masses m 1 and m 2 distance r apart F = Gm 1 m 2/r 2 m 1 m 2 Looking at the force on m 1 due to m 2, F = gm 1 F = Gm 1 m 2/r 2 = gm 1 g (field due to m 2) = Gm 2/r 2

Gravitational field around a point I told you, for any mass planet; If we

Gravitational field around a point I told you, for any mass planet; If we have two masses m 1 and m 2 distance r apart g = Gmp F = Gm 1 m 2/r 2 r p 2 m 2 for a Don’t forget that nontopoint Looking at the force on m 1 due m 2, Fmass, = gmr 1 is the distance to the centre of mass F = Gm 1 m 2/r 2 = gm 1 g (field due to m 2) = Gm 2/r 2

Gravitational field is a vector, and any calculations regarding fields (especially involving adding the

Gravitational field is a vector, and any calculations regarding fields (especially involving adding the fields from more than one mass) must use vector addition. Field here due to both masses? m 1 m 2

Gravitational field is a vector, and any calculations regarding fields (especially involving adding the

Gravitational field is a vector, and any calculations regarding fields (especially involving adding the fields from more than one mass) must use vector addition. Field due to m 1 Field here due to both masses? m 2

Gravitational field is a vector, and any calculations regarding fields (especially involving adding the

Gravitational field is a vector, and any calculations regarding fields (especially involving adding the fields from more than one mass) must use vector addition. Field due to m 1 Field due to m 2

Gravitational field is a vector, and any calculations regarding fields (especially involving adding the

Gravitational field is a vector, and any calculations regarding fields (especially involving adding the fields from more than one mass) must use vector addition. Field due to m 1 Field due to m 2 Resultant Field m 1 m 2

Gravitational field patterns A gravitational field can be represented by lines and arrows on

Gravitational field patterns A gravitational field can be represented by lines and arrows on a diagram, in a similar ways to magnetic field lines.

Gravitational field patterns A gravitational field can be represented by lines and arrows on

Gravitational field patterns A gravitational field can be represented by lines and arrows on a diagram, in a similar ways to magnetic field lines. The closer the lines are together, the stronger the force felt. This is an example of a radial field Note, gravity is ALWAYS attractive

Field around a charged metal sphere E = 0 inside the sphere

Field around a charged metal sphere E = 0 inside the sphere

Field around a uniform spherical mass

Field around a uniform spherical mass

Field close to the earth’s surface Uniform

Field close to the earth’s surface Uniform